# Model_Name
`hc`: thickness of methane clathrate
`dimp`: diameter of impactor

# iSALE_inputs; *.inp
input files for the model
- asteroid_res*m.inp
- material.inp: cases without ocean (dimp1.5--4km)
- material_wocean.inp: cases with ocean (dimp5--25km)
- temperature_profile*.txt
To use these for `LAYTPROF: USER` case, rename or link them.
Reference for these temperature profiles: 
Kalousova, K. & Sotin, C. The Insulating Effect of Methane Clathrate Crust on Titan's Thermal Evolution. Geophys. Res. Lett. 47, e2020GL087481 (2020). doi:10.1029/2020GL087481.

# iSALE_outputs; *.dat
Please connect *_00, *_01, and *_?? by `cat FILE_* >> FILE`.
*.dat.t0_* and *.dat.t1_* are continuous.

Note some files are duplicate of previous work:
Wakita, S., Johnson, B. C., Soderblom, J. M., Shah, J., Neish, C. D., & Steckloff, J. K. (2023). Modeling the Formation of Selk Impact Crater on Titan Implications for Dragonfly. The Planetary Science Journal, 4 (3), 51. doi:10.3847/PSJ/acbe40
"Replication Data for: Modeling the formation of Selk impact crater on Titan: Implications for Dragonfly", https://doi.org/10.7910/DVN/XEGCCO

